Subscribe free to our newsletters via your
. 24/7 Space News .




SOLAR SCIENCE
New Research Settles Years Debate Over Diffuse Aurora
by Staff Writers
London, UK (SPX) Oct 22, 2010


The 'aurora australis' (known as the southern lights) seen in Antarctica. The 'aurora australis' look like fiery, moving curtains of colourful light and can be seen by the naked eye whereas the diffuse aurora is much fainter (viewed via satellite), but is more extensive.

New space research published this week (Thursday 21 October) in the journal Nature, has settled decades of scientific debate. Researchers from the University of California (UCLA) and British Antarctic Survey (BAS) have found the final link between electrons trapped in space and the glow of light from the upper atmosphere known as the diffuse aurora.

The research will help us understand 'space weather', with benefits for the satellite, power grid and aviation industries, and how space storms affect the Earth's atmosphere from the top down.

Scientists have long understood that the 'diffuse aurora' is caused by electrons striking the upper atmosphere. However, the electrons are normally trapped much higher up in the Earth's magnetic field through a long chain of events starting with the Sun. The problem is to understand how these electrons reach the atmosphere.

Since the 1970s scientists have debated whether very low frequency (VLF) radio waves could scatter the trapped electrons into the atmosphere. Two types of VLF waves were identified in space as the possible cause of the 'diffuse aurora', but despite years of argument and research no conclusive result had been possible.

The new research shows, without doubt, that VLF waves known as 'chorus' are responsible; so-called since the signals detected by ground-based recording equipment sound like the bird's dawn chorus when played back through a loud speaker.

Through detailed analysis of satellite data the authors were able to calculate the effects on the trapped electrons and identify which radio waves were causing the scattering.

Lead author Professor Richard Thorne from UCLA said, "The breakthrough came when we realised that the electrons being lost from space to the Earth's atmosphere were leaving a signature, effectively telling a story about how they were being scattered.

We could then analyse our satellite data on the two types of VLF waves and by running calculations on them - including the rate at which the electrons were being lost to the Earth's atmosphere - we could clearly see that chorus waves were the cause of the scattering."

Professor Richard Horne from British Antarctic Survey said, "Our finding is an important one because it will help scientists to understand how the diffuse aurora leads to changes in the chemistry of the Earth's upper atmosphere, including effects on ozone at high altitude, which may affect temperature right through the atmosphere.

"We are also including the VLF waves into computer models to help predict 'space weather' which not only affects satellites and power grids, but also the accuracy of GPS navigation and high frequency radio communications with aircraft on polar routes."

The 'diffuse aurora', is not the same as the 'discrete aurora' known as the northern and southern lights. 'Discrete aurora' look like fiery moving curtains of colourful light and can be seen by the naked eye, whereas the diffuse aurora is much fainter but more extensive. The 'diffuse aurora', which typically accounts for three-quarters of the energy input into the upper atmosphere at night, varies according to the season and the 11 year solar cycle.

*Chorus waves: Very low frequency radio waves coming from space and first detected on the ground. So-called because when played back through a loud speaker they sound like the bird's dawn chorus

*Diffuse aurora: caused when electrons that are trapped in the Earth's magnetic field are funnelled towards the polar atmosphere. Light is emitted when the electrons collide with neutral atoms in the upper atmosphere. The diffuse aurora is not generally visible to the naked eye but is well captured in satellite images.

*Discrete aurora: known as the Aurora Borealis at the North Pole (above the Arctic circle) and Aurora Australis at the South Pole (above Antarctica). They look like fiery, moving curtains of colourful light and can be seen by the naked eye whereas the diffuse aurora is much fainter but is more extensive and can cover the whole sky.

Thorne, R. M., Ni, B., Tao, X., Horne, R. B., and Meredith N. P., Scattering by chorus waves as the dominant cause of diffuse auroral precipitation, Nature, doi:10.1038/nature09467 (2010).

.


Related Links
UK at Antarctica
Solar Science News at SpaceDaily






Comment on this article via your Facebook, Yahoo, AOL, Hotmail login.

Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle








SOLAR SCIENCE
Study Sheds New Light On How The Sun Affects The Earth's Climate
London, UK (SPX) Oct 11, 2010
The Sun's activity has recently affected the Earth's atmosphere and climate in unexpected ways, according to a new study published in the journal Nature. The study, by researchers from Imperial College London and the University of Colorado, shows that a decline in the Sun's activity does not always mean that the Earth becomes cooler. It is well established that the Sun's activity waxes and ... read more


SOLAR SCIENCE
LRO Detects Surprising Gases In LCROSS Lunar Impact Plume

Moon's 'treasure chest' includes silver : study

LRO Supports Historic Lunar Impact Mission

NASA to buy private moon data

SOLAR SCIENCE
Curiosity Builds A New Mars Rover

Opportunity's Eastward View After Sol 2382 Drive

The Continuing Controversy Of The Mars Meteorite

Testing The Exomars Rover In Mars-Like Conditions

SOLAR SCIENCE
Cosmonaut food prices skyrocket due to inflation: official

Study: Space tourism could pollute skies

Runway unveiled for world's first 'tourist' spaceship

NASA Space Technology Could Transform Life On Earth

SOLAR SCIENCE
The International Future In Space

International Crews for Shenzhou

China Eyes Extended Mission Beyond Moon

China's second lunar probe enters moon's orbit: state media

SOLAR SCIENCE
New International Standard For Spacecraft Docking

Counting Down For ESA MagISStra Mission To Space Station

Glamorous spy sees Russian rocket blast off for ISS

Russian rocket blasts off carrying three astronauts to ISS

SOLAR SCIENCE
Hylas-1 Satellite Readied For Launch From European Spaceport

ILS Proton Successfully Launches XM-5 Satellite

Ariane Moves Into Final Phase Of Globalstar Soyuz 2 Launch Campaign

Arianespace Hosts Meeting Of Launch System Manufacturers

SOLAR SCIENCE
Astronomers Find Weird, Warm Spot On An Exoplanet

New techniqe aiding planet searches

Planet Hunters No Longer Blinded By The Light

How To Weigh A Star Using A Moon

SOLAR SCIENCE
NASA Open Government Summit Emphasized Data Exchange

HP unveils 'Slate 500' tablet computer for professionals

Japan's rare earth minerals may run out by March: govt

Japan and Vietnam to jointly develop rare earth: report




The content herein, unless otherwise known to be public domain, are Copyright 1995-2014 - Space Media Network. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA Portal Reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement